Constraints on coronal outflow velocities derived from UVCS Doppler dimming measurements and in-situ charge state data

Space Science Reviews

Volumn 87, Issue 1-2, 1999, Pages 311-314

  Strachan, Leonard ^a   Ko, Y K ^a   Panasyuk, A V ^a   Dobrzycka, D ^a   Kohl, J L ^a   Romoli, M ^b   Noci, G ^b   Gibson, S E ^c   Biesecker, D A ^c,d  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b UNIVERSITY OF FLORENCE   (Italy)

^c NASA GODDARD SPACE FLIGHT CENTER   (United States)

^d UNIVERSITY OF BIRMINGHAM   (United Kingdom)

Author keywords

Corona; Line profiles; Solar wind; Spectroscopy; UV radiation

Indexed keywords

EID: 0009878644     PISSN: 00386308     EISSN: None     Source Type: Journal    
DOI: 10.1007/978-94-015-9167-6_52     Document Type: Article

References (7)

1. Guhathakurta, M., and Fisher, R.: 1998, Astrophys. J., 499, L215.
2. Hundhausen, A. J.: 1972, Coronal Expansion and Solar Wind, (Springer-Verlag, New York), p. 114.
3. Ko, Y.-K., Fisk, L. A., Geiss, J., Gloeckler, G., and Guhathakurta, M.: 1997, Solar Phys., 171, 345.
4. Kohl, J. L., et al.: 1998, Astrophys. J., 501, L127.
5. Panasyuk, A. V.: 1999, J. Geophys. Res., in press.
6. Strachan, L., Kohl, J. L., Weiser, H., Withbroe, G. L., and Munro, R. H.: 1993, Astrophys. J., 412, 410.
7. Withbroe, G. L., Kohl, J. L., Weiser, H., and Munro, R. H.: 1982, Space Sci. Rev., 33, 17.